Portable mass spectrometry system: instrumentation, applications, and path to 'omics analysis
Mass spectrometry (MS) is an information rich analytical technique and plays a key role in
various 'omics studies. Standard mass spectrometers are bulky and operate at high vacuum …
various 'omics studies. Standard mass spectrometers are bulky and operate at high vacuum …
Interaction of the solar wind with comets: a Rosetta perspective
KH Glassmeier - … Transactions of the Royal Society A …, 2017 - royalsocietypublishing.org
The Rosetta mission provides an unprecedented possibility to study the interaction of
comets with the solar wind. As the spacecraft accompanies comet 67P/Churyumov …
comets with the solar wind. As the spacecraft accompanies comet 67P/Churyumov …
Interplanetary coronal mass ejection observed at STEREO‐A, Mars, comet 67P/Churyumov‐Gerasimenko, Saturn, and New Horizons en route to Pluto: Comparison of …
O Witasse, B Sánchez‐Cano, ML Mays… - Journal of …, 2017 - Wiley Online Library
We discuss observations of the journey throughout the Solar System of a large
interplanetary coronal mass ejection (ICME) that was ejected at the Sun on 14 October …
interplanetary coronal mass ejection (ICME) that was ejected at the Sun on 14 October …
Ionospheric plasma of comet 67P probed by Rosetta at 3 AU from the Sun
M Galand, KL Héritier, E Odelstad… - Monthly Notices of …, 2016 - academic.oup.com
We propose to identify the main sources of ionization of the plasma in the coma of comet
67P/Churyumov-Gerasimenko at different locations in the coma and to quantify their relative …
67P/Churyumov-Gerasimenko at different locations in the coma and to quantify their relative …
Birth of a comet magnetosphere: A spring of water ions
The Rosetta mission shall accompany comet 67P/Churyumov-Gerasimenko from a
heliocentric distance of> 3.6 astronomical units through perihelion passage at 1.25 …
heliocentric distance of> 3.6 astronomical units through perihelion passage at 1.25 …
Dynamical features and spatial structures of the plasma interaction region of 67P/Churyumov–Gerasimenko and the solar wind
C Koenders, KH Glassmeier, I Richter… - Planetary and Space …, 2015 - Elsevier
In the advent of the Rosetta arrival at the comet 67P/Churyumov–Gerasimenko, we present
a global 3D hybrid simulation model of the cometary plasma interaction which resolves the …
a global 3D hybrid simulation model of the cometary plasma interaction which resolves the …
Evolution of the ion environment of comet 67P/Churyumov-Gerasimenko-Observations between 3.6 and 2.0 AU
Context. The Rosetta spacecraft is escorting comet 67P/Churyumov-Gerasimenko from a
heliocentric distance of> 3.6 AU, where the comet activity was low, until perihelion at 1.24 …
heliocentric distance of> 3.6 AU, where the comet activity was low, until perihelion at 1.24 …
RPC observation of the development and evolution of plasma interaction boundaries at 67P/Churyumov-Gerasimenko
One of the primary objectives of the Rosetta Plasma Consortium, a suite of five plasma
instruments on-board the Rosetta spacecraft, is to observe the formation and evolution of …
instruments on-board the Rosetta spacecraft, is to observe the formation and evolution of …
The birth and growth of a solar wind cavity around a comet – Rosetta observations
The Rosetta mission provided detailed observations of the growth of a cavity in the solar
wind around comet 67P/Churyumov–Gerasimenko. As the comet approached the Sun, the …
wind around comet 67P/Churyumov–Gerasimenko. As the comet approached the Sun, the …
Evolution of the ion environment of comet 67P during the Rosetta mission as seen by RPC-ICA
Rosetta has followed comet 67P from low activity at more than 3.6 au heliocentric distance to
high activity at perihelion (1.24 au) and then out again. We provide a general overview of the …
high activity at perihelion (1.24 au) and then out again. We provide a general overview of the …